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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/634
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dc.contributor.authorDatta, B-
dc.contributor.authorKapoor, R. C-
dc.date.accessioned2005-12-07T04:31:03Z-
dc.date.available2005-12-07T04:31:03Z-
dc.date.issued1984-12-
dc.identifier.citationBASI, Vol. 12, No. 4, pp. 343-349en
dc.identifier.urihttp://hdl.handle.net/2248/634-
dc.description.abstractGeneral relativistic effects of rotation on the structure and surface emission of the fast pulsar PSR 1937 + 214 are illustrated using a rotationally perturbed interior spherical metric. The results are found to differ markedly from those derived on the basis of simple spherical models, and are expected to be generally valid for the class of fast pulsars.en
dc.format.extent546521 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectGeneral relativityen
dc.subjectNeutron star structureen
dc.subjectFast Pulsarsen
dc.subjectRedshiften
dc.titleGeneral Relativistic effects of rotation on the structure and surface redshift of fast pulsarsen
dc.typeArticleen
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